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Io

Io is the innermost of Jupiter’s four Galilean moons and the third-largest moon of Jupiter.

By Ethan Anderson| Reviewed by Olivia Bennett, Standards & Fact-Checking Lead| Updated July 26, 2026|2 min read| Fact-checked

Io is the innermost of Jupiter’s four Galilean moons and the third-largest moon of Jupiter. It is the most volcanically active world in the Solar System, with hundreds of volcanoes driven by tidal heating from Jupiter and neighbouring moons. Io was discovered by Galileo Galilei in 1610.

Discovery and naming

Io was discovered by Galileo Galilei in 1610 during his observations of Jupiter’s moons. The name Io comes from Greek mythology and was later adopted as the moon’s standard name.

Orbit and physical characteristics

Io orbits very close to Jupiter and completes one orbit in about 42.5 hours. It is slightly larger than Earth’s Moon and is among the densest moons in the Solar System.

Volcanism and geology

Io is the most volcanically active world in the Solar System. Its surface is continually resurfaced by volcanic eruptions, lava flows, and sulfurous deposits, leaving relatively few impact craters.

Atmosphere and surface composition

Io has a very thin atmosphere, mainly composed of sulfur dioxide. Its surface contains sulfur and silicate materials, producing distinctive yellow, red, white, black, and green colouring.

Key facts

  • Io is one of Jupiter’s four Galilean moons, along with Europa, Ganymede, and Callisto.
  • It is the innermost of the Galilean moons and the third-largest moon of Jupiter.
  • Io’s surface is shaped by extreme volcanism, with hundreds of volcanoes and active lava fountains.
  • Its activity is powered by tidal heating caused by gravitational interactions with Jupiter, Europa, and Ganymede.
  • Io was first observed by Galileo Galilei on 8 January 1610.
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Canadian context

Io is a major object of interest for Canadian astronomy education and public science outreach because it is a nearby, well-studied example of tidal heating and active volcanism in the Solar System.

Frequently asked questions

What is Io?
Io is a natural satellite of Jupiter and one of the four Galilean moons.
Why is Io so volcanically active?
Io’s volcanism is driven by tidal heating from Jupiter’s gravity and gravitational interactions with Europa and Ganymede.
Who discovered Io?
Io was discovered by Galileo Galilei on 8 January 1610.
How big is Io?
Io is about 3,643 km in diameter, slightly larger than Earth’s Moon.
Does Io have an atmosphere?
Yes, but it is extremely thin and is composed mainly of sulfur dioxide.

References

  1. NASA Sciencehttps://science.nasa.gov/jupiter/jupiter-moons/io/facts/
    Supports: Discovery date, volcanic activity, Galilean moon status, size relative to Earth's Moon, orbital position.
  2. NASA Sciencehttps://science.nasa.gov/jupiter/jupiter-moons/io/
    Supports: Most volcanically active world, tidal heating explanation, lava fountains, lava lakes, general overview.
  3. The Planetary Societyhttps://www.planetary.org/worlds/io
    Supports: Innermost Galilean moon, volcanic activity, atmosphere composition, orbital and physical context.
  4. Encyclopaedia Britannicahttps://www.britannica.com/place/Io-satellite-of-Jupiter
    Supports: Discovery by Galileo, innermost Galilean moon, naming context, volcanic activity.
  5. European Space Agencyhttps://sci.esa.int/web/hubble/-/39830-the-volcanic-moon-io
    Supports: Sulfur dioxide frost, extremely tenuous atmosphere, discovery context, volcanism observations.